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Both sides previous revision Previous revision Next revision | Previous revision Next revision Both sides next revision | ||
herschel [2018/10/09 15:10] Déborah Paradis |
herschel [2021/01/27 10:12] Déborah Paradis |
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The photometric bands are centered at 70, 100 and 160 microns for PACS, and at 250, 350 and 500 microns for SPIRE, with an angular resolution going from 5 arcsec to 37 arcsec. | The photometric bands are centered at 70, 100 and 160 microns for PACS, and at 250, 350 and 500 microns for SPIRE, with an angular resolution going from 5 arcsec to 37 arcsec. | ||
- | CADE currently only serves SPIRE photometric data for each Key-Programs. Healpix maps at 250 microns and 350 microns have been smoothed to 37 arcsec. | + | CADE currently only serves SPIRE photometric data for each Key-Programs. Healpix maps at 250 microns and 350 microns have been smoothed to 37 arcsec. We also provide Healpix maps at 4' angular resolution. |
The units of the Healpix maps are MJy/sr. | The units of the Healpix maps are MJy/sr. | ||
Line 25: | Line 25: | ||
|[[Herschel Galactic Cold Cores|Galactic Cold Cores (PI: M. Juvela & I. Ristorcelli)]]|\\ | |[[Herschel Galactic Cold Cores|Galactic Cold Cores (PI: M. Juvela & I. Ristorcelli)]]|\\ | ||
|[[Herschel GOODS|GOODS- The Great Observatories Origins Deep Survey: far-infrared imaging with Herschel (PI: D. Elbaz)]]| \\ | |[[Herschel GOODS|GOODS- The Great Observatories Origins Deep Survey: far-infrared imaging with Herschel (PI: D. Elbaz)]]| \\ | ||
+ | |[[Herschel Gould Belt|Gould Belt- Probing the origin of the stellar initial mass function: A wide-field Herschel photometric survey of nearby star-forming cloud complexes (PI: P. André)]]| \\ | ||
|[[Herschel H-atlas|H-ATLAS- The Herschel Thousand Degree Survey (PI: S. Eales)]]|\\ | |[[Herschel H-atlas|H-ATLAS- The Herschel Thousand Degree Survey (PI: S. Eales)]]|\\ | ||
|[[Herschel Lensing Survey|Herschel Lensing Survey (PI: E. Egami)]]|\\ | |[[Herschel Lensing Survey|Herschel Lensing Survey (PI: E. Egami)]]|\\ |